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Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies

T. Tal, A. Dekel, P. Oesch, A. Muzzin, G. Brammer, P. van Dokkum, M. Franx, G. Illingworth, J. Leja, D. Magee, D. Marchesini, I. Momcheva, E. Nelson, S. Patel, R. Quadri, H. Rix, R. Skelton, D. Wake, и K. Whitaker. (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.

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Anthony Illingworth

Christoph Garth

Hartmut Garth

Herbert Garth

Julia Gärth

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Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$S. Schouws, M. Stefanon, R. Bouwens, R. Smit, J. Hodge, I. Labbé, H. Algera, L. Boogaard, S. Carniani, Y. Fudamoto и 6 other автор(ы). (2021)cite arxiv:2105.12133Comment: 21 pages, 12 figures, 2 tables. Submitted to ApJ.The Evolution of Mass-size Relation for Lyman Break Galaxies From z=1 to z=7M. Mosleh, R. Williams, M. Franx, V. Gonzalez, R. Bouwens, P. Oesch, I. Labbe, G. Illingworth, и M. Trenti. (2012)cite arxiv:1207.6634Comment: Accepted for publication in The Astrophysical Journal Letters.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift GalaxiesN. Reddy, P. Oesch, R. Bouwens, M. Montes, G. Illingworth, C. Steidel, P. van Dokkum, H. Atek, M. Carollo, A. Cibinel и 6 other автор(ы). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?R. Naidu, P. Oesch, D. Setton, J. Matthee, C. Conroy, B. Johnson, J. Weaver, R. Bouwens, G. Brammer, P. Dayal и 15 other автор(ы). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.Dark-ages Reionization and Galaxy Formation Simulation XX. The Ly$\alpha$ IGM transmission properties and environment of bright galaxies during the Epoch of ReionizationY. Qin, J. Wyithe, P. Oesch, G. Illingworth, E. Leonova, S. Mutch, и R. Naidu. (2021)cite arxiv:2108.03675Comment: 10 pages, 3 figures, submitted to MNRAS, comments are welcome.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxiesT. Tal, A. Dekel, P. Oesch, A. Muzzin, G. Brammer, P. van Dokkum, M. Franx, G. Illingworth, J. Leja, D. Magee и 9 other автор(ы). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.Measurement of rotation in two galaxies in the Epoch of Reionization from ALMA-detected CII emissionR. Smit, R. Bouwens, S. Carniani, P. Oesch, I. Labbé, G. Illingworth, P. van der Werf, L. Bradley, V. Gonzalez, J. Hodge и 2 other автор(ы). (2017)cite arxiv:1706.04614Comment: 13 pages, 5 figues, 1 table, submitted.

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